Zobrazeno 1 - 10
of 321
pro vyhledávání: '"Patten B"'
Publikováno v:
In Radiography February 2021 27(1):156-161
Autor:
Dong, Subo, Udalski, A., Gould, A., Reach, W. T., Christie, G. W., Boden, A. F., Bennett, D. P., Fazio, G., Griest, K., Szymanski, M. K., Kubiak, M., Soszynski, I., Pietrzynski, G., Szewczyk, O., Wyrzykowski, L., Ulaczyk, K., Wieckowski, T., Paczynski, B., DePoy, D. L., Pogge, R. W., Preston, G. W., Thompson, I. B., Patten, B. M.
Publikováno v:
Astrophys.J.664:862-878,2007
We combine Spitzer and ground-based observations to measure the microlens parallax of OGLE-2005-SMC-001, the first such space-based determination since S. Refsdal proposed the idea in 1966. The parallax measurement yields a projected velocity \tilde
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702240
Autor:
Luhman, K. L., Patten, B. M., Marengo, M., Schuster, M. T., Hora, J. L., Ellis, R. G., Stauffer, J. R., Sonnett, S. M., Winston, E., Gutermuth, R. A., Megeath, S. T., Backman, D. E., Henry, T. J., Werner, M. W., Fazio, G. G.
Publikováno v:
Astrophys.J.654:570-579,2006
We report the discovery of T dwarf companions to the nearby stars HN Peg (G0V, 18.4 pc, ~0.3 Gyr) and HD 3651 (K0V, 11.1 pc, ~7 Gyr). During an ongoing survey of 5'x5' fields surrounding stars in the solar neighborhood with IRAC aboard the Spitzer Sp
Externí odkaz:
http://arxiv.org/abs/astro-ph/0609464
Autor:
Morales-Calderon, M., Stauffer, J. R., Kirkpatrick, J. Davy, Carey, S., Gelino, C. R., Navascues, D. Barrado y, Rebull, L., Lowrance, P., Marley, M. S., Charbonneau, D., Patten, B. M., Megeath, S. T., Buzasi, D.
Publikováno v:
Astrophys.J.653:1454-1463,2006
We have conducted a photometric monitoring program of 3 field late-L brown dwarfs looking for evidence of non-axisymmetric structure or temporal variability in their photospheres. The observations were performed using Spitzer/IRAC 4.5 and 8 micron ba
Externí odkaz:
http://arxiv.org/abs/astro-ph/0607537
Autor:
Bensch, F., Melnick, G. J., Neufeld, D. A., Harwit, M., Snell, R. L., Patten, B. M., Tolls, V.
On 4 July 2005 at 5:52 UT the Deep Impact mission successfully completed its goal to hit the nucleus of 9P/Tempel 1 with an impactor, forming a crater on the nucleus and ejecting material into the coma of the comet. NASA's Submillimeter Wave Astronom
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606045
Autor:
Snell, R. L., Howe, J. E., Ashby, M. L. N., Bergin, E. A., Chin, G., Erickson, N. R., Goldsmith, P. F., Harwit, M., Kleiner, S. C., Koch, D. G., Neufeld, D. A., Patten, B. M., Plume, R., Schieder, R., Stauffer, J. R., Tolls, V., Wang, Z., Winnewisser, G., Zhang, Y. F., Melnick, G. J.
Publikováno v:
ApJ (Letters), 539, L101 (2000)
We present Submillimeter Wave Astronomy Satellite (SWAS) observations of the 1_{10}-1_{01} transition of ortho-water at 557 GHz toward 12 molecular cloud cores. The water emission was detected in NGC 7538, Rho Oph A, NGC 2024, CRL 2591, W3, W3(OH), M
Externí odkaz:
http://arxiv.org/abs/astro-ph/0010393
Autor:
Snell, R. L., Howe, J. E., Ashby, M. L. N., Bergin, E. A., Chin, G., Erickson, N. R., Goldsmith, P. F., Harwit, M., Kleiner, S. C., Koch, D. G., Neufeld, D. A., Patten, B. M., Plume, R., Schieder, R., Stauffer, J. R., Tolls, V., Wang, Z., Winnewisser, G., Zhang, Y. F., Melnick, G. J.
Publikováno v:
ApJ (Letters), 539, L97 (2000)
We present a 17-point map of the M17SW cloud core in the 1_{10}-1_{01} transition of ortho-water at 557 GHz obtained with the Submillimeter Wave Astronomy Satellite. Water emission was detected in 11 of the 17 observed positions. The line widths of t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0010392
Autor:
Howe, J. E., Ashby, M. L. N., Bergin, E. A., Chin, G., Erickson, N. R., Goldsmith, P. F., Harwit, M., Hollenbach, D. J., Kaufman, M. J., Kleiner, S. C., Koch, D. G., Neufeld, D. A., Patten, B. M., Plume, R., Schieder, R., Snell, R. L., Stauffer, J. R., Tolls, V., Wang, Z., Winnewisser, G., Zhang, Y. F., Melnick, G. J.
Publikováno v:
ApJ (Letters), 539, L137 (2000)
We mapped a 13 by 22 pc region in emission from 492 GHz [C I] and, for the first time, 551 GHz ^{13}CO(5-4) in the giant molecular cloud M17SW, using the Submillimeter Wave Astronomy Satellite. The morphologies of the [C I] and ^{13}CO emission are s
Externí odkaz:
http://arxiv.org/abs/astro-ph/0010394
Autor:
Snell, R. L., Howe, J. E., Ashby, M. L. N., Bergin, E. A., Chin, G., Erickson, N. R., Goldsmith, P. F., Harwit, M., Kleiner, S. C., Koch, D. G., Neufeld, D. A., Patten, B. M., Plume, R., Schieder, R., Stauffer, J. R., Tolls, V., Wang, Z., Winnewisser, G., Zhang, Y. F., Melnick, G. J.
Publikováno v:
ApJ (Letters), 539, L93 (2000)
We have used the Submillimeter Wave Astronomy Satellite to map the ground-state 1_{10}-1_{01} transition of ortho-water at 557 GHz in the Orion molecular cloud. Water emission was detected in Orion over an angular extent of about 20 arcmin, or nearly
Externí odkaz:
http://arxiv.org/abs/astro-ph/0010391
Autor:
Meech, K. J., Ageorges, N., Arpigny, C., Ates, A., Aycock, J., Bagnulo, S., Bailey, J., Barber, R., Barrera, L., Barrena, R., Bauer, J. M., Belton, M. J. S., Bensch, F., Bhattacharya, B., Biver, N., Blake, G., Bockelée-Morvan, D., Boehnhardt, H., Bonev, B. P., Bonev, T., Buie, M. W., Burton, M. G., Butner, H. M., Cabanac, R., Campbell, R., Campins, H., Capria, M. T., Carroll, T., Chaffee, F., Charnley, S. B., Cleis, R., Coates, A., Cochran, A., Colom, P., Conrad, A., Coulson, I. M., Crovisier, J., deBuizer, J., Dekany, R., de Léon, J., Russo, N. Dello, Delsanti, A., DiSanti, M., Drummond, J., Dundon, L., Etzel, P. B., Farnham, T. L., Feldman, P., Fernández, Y. R., Filipovic, M. D., Fisher, S., Fitzsimmons, A., Fong, D., Fugate, R., Fujiwara, H., Fujiyoshi, T., Furusho, R., Fuse, T., Gibb, E., Groussin, O., Gulkis, S., Gurwell, M., Hadamcik, E., Hainaut, O., Harker, D., Harrington, D., Harwit, M., Hasegawa, S., Hergenrother, C. W., Hirst, P., Hodapp, K., Honda, M., Howell, E. S., Hutsemékers, D., Iono, D., Jackson, W., Jehin, E., Jiang, Z. J., Jones, G. H., Jones, P. A., Kadono, T., Kamath, U. W., Käufl, H. U., Kasuga, T., Kawakita, H., Kelley, M. S., Kerber, F., Kidger, M., Kinoshita, D., Knight, M., Lara, L., Larson, S. M., Lederer, S., Levasseur-Regourd, A. C., Li, J. Y., Licandro, J., Lisse, C. M., LoCurto, G., Lovell, A. J., Lowry, S. C., Lyke, J., Lynch, D., Ma, J., Magee-Sauer, K., Maheswar, G., Manfroid, J., Marco, O., Martin, P., Melnick, G., Miller, S., Miyata, T., Moriarty-Schieven, G. H., Moskovitz, N., Mueller, B. E. A., Mumma, M. J., Muneer, S., Neufeld, D. A., Ootsubo, T., Osip, D., Pandea, S. K., Pantin, E., Paterno-Mahler, R., Patten, B., Penprase, B. E., Peck, A., Petitas, G., Pinilla-Alonso, N., Pittichova, J., Pompei, E., Prabhu, T. P., Qi, C., Rao, R., Rauer, H., Reitsema, H., Rodgers, S. D., Rodriguez, P., Ruane, R., Ruch, G., Rujopakarn, W., Sahu, D. K., Sako, S., Sakon, I., Samarasinha, N., Sarkissian, J. M., Saviane, I., Schirmer, M., Schultz, P., Schulz, R., Seitzer, P., Sekiguchi, T., Selman, F., Serra-Ricart, M., Sharp, R., Snell, R. L., Snodgrass, C., Stallard, T., Stecklein, G., Sterken, C., Stüwe, J. A., Sugita, S., Sumner, M., Suntzeff, N., Swaters, R., Takakuwa, S., Takato, N., Thomas-Osip, J., Thompson, E., Tokunaga, A. T., Tozzi, G. P., Tran, H., Troy, M., Trujillo, C., Van Cleve, J., Vasundhara, R., Vazquez, R., Vilas, F., Villanueva, G., von Braun, K., Vora, P., Wainscoat, R. J., Walsh, K., Watanabe, J., Weaver, H. A., Weaver, W., Weiler, M., Weissman, P. R., Welsh, W. F., Wilner, D., Wolk, S., Womack, M., Wooden, D., Woodney, L. M., Woodward, C., Yamashita, T., Yang, B., Yokogawa, S., Zook, A. C., Zauderer, A., Zhao, X., Zhou, X.
Publikováno v:
Science, 2005 Oct . 310(5746), 265-269.
Externí odkaz:
https://www.jstor.org/stable/3842647